The classical model of the formation of Earth’s magnetic field raised a major paradox. For the geodynamo to work, the Earth would have had to be totally molten four billion years ago, and its core would have had to slowly cool from around 6800 °C at that time to 3800 °C today. However, recent modeling of the early evolution of the internal temperature of the planet, together with geochemical studies of the composition of the oldest carbonatites and basalts, do not support such cooling. With such high temperatures being ruled out, the researchers propose another source of energy in their study.
The Earth has a slightly flattened shape and rotates about an inclined axis that wobbles around the poles. Its mantle deforms elastically due to tidal effects caused by the Moon. The researchers show that this effect could continuously stimulate the motion of the liquid iron alloy making up the outer core, and in return generate Earth’s magnetic field. The Earth continuously receives 3,700 billion watts of power through the transfer of the gravitational and rotational energy of the Earth-Moon-Sun system, and over 1,000 billion watts is thought to be available to bring about this type of motion in the outer core. This energy is enough to generate the Earth’s magnetic field, which together with the Moon, resolves the major paradox in the classical theory. The effect of gravitational forces on a planet’s magnetic field has already been well documented for two of Jupiter’s moons, Io and Europa, and for a number of exoplanets.
Since neither the Earth’s rotation around its axis, nor the direction of its axis, nor the Moon’s orbit are perfectly regular, their combined effect on motion in the core is unstable and can cause fluctuations in the geodynamo. This process could account for certain heat pulses in the outer core and at its boundary with the Earth’s mantle.
Over the course of time, this may have led to peaks in deep mantle melting and possibly to major volcanic events at the Earth’s surface. This new model shows that the Moon’s effect on the Earth goes well beyond merely causing tides.
 At the Laboratoire Magmas et Volcans (CNRS/IRD/Université Blaise Pascal), part of the Observatoire de Physique du Globe de Clermont-Ferrand, the Institut de Recherche sur les Phénomènes Hors-équilibre (CNRS/Aix-Marseille Université/Ecole Centrale Marseille) and the Institut de Recherche en Astrophysique et Planétologie (CNRS/Université Toulouse III — Paul Sabatier).